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Infrared companions to pre-main sequence stars

✍ Scribed by H. Zinnecker; A. Chelli; L. Carrasco; I. Cruz-Gonzalez; C. Perrier


Publisher
Springer Netherlands
Year
1988
Tongue
English
Weight
43 KB
Volume
142
Category
Article
ISSN
0004-640X

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Pre-Main-Sequence stars with masses between 2 and 5 M e (Herbig Ae/Be stars) have radiative subphotospheric envelopes. However, they possess strong stellar winds and show definite signs of activity which could be linked to surface magnetic field. Therefore, they must lose angular momentum at a signi